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arXiv · 0901.0849

A TeV-scale model for neutrino mass, DM and baryon asymmetry

Mayumi Aoki·Shinya Kanemura·Osamu Seto
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Abstract

We discuss a model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the physics at TeV scales. Tiny neutrino masses are generated at the three loop level due to the exact $Z_2$ symmetry, by which the stability of the dark matter candidate is also guaranteed. The extra Higgs doublet is required not only for the tiny neutrino masses but also for successful electroweak baryogenesis. The model provides various discriminative predictions especially in charged Higgs phenomenology.

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Mayumi Aoki, Shinya Kanemura, Osamu Seto. 2009-01-07. A TeV-scale model for neutrino mass, DM and baryon asymmetry. https://arxiv.org/abs/0901.0849

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